SDO HMI 2014-07-04 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.33 | 0.00 | 14.35 | 8.27 | 262.80 | -17.12 | 69.70 | 0.3066 | 575.9 | 558.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.44 | 278.94 | -0.98 | 75.46 | 0.0176 | -1033.0 | -843.9 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 6.09 | 278.21 | -1.71 | 30.37 | 0.0590 | -689.0 | -576.7 | |
| 0.00 | 2.00 | 0.00 | 1.01 | 9.36 | 269.65 | -10.27 | 58.38 | 0.2075 | 1014.0 | 865.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 8.56 | 269.08 | -10.84 | 63.07 | 0.2096 | 843.0 | 713.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 9.59 | 265.69 | -14.23 | 64.97 | 0.2687 | 930.0 | 639.9 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 8.48 | 265.10 | -14.82 | 69.61 | 0.2711 | 906.0 | 739.5 | |
| 0.00 | 8.27 | 0.00 | 4.34 | 8.85 | 261.28 | -18.64 | 72.17 | 0.3332 | 803.0 | 721.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 9.06 | 260.91 | -19.01 | 71.87 | 0.3399 | 771.0 | 646.4 | |
| 0.00 | 2.00 | 0.00 | 1.06 | 8.96 | 260.33 | -19.59 | 72.61 | 0.3486 | 863.0 | 637.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.78 | 260.24 | -19.68 | 73.19 | 0.3492 | 686.0 | 576.3 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 7.70 | 258.55 | -21.37 | 77.13 | 0.3719 | 819.0 | 668.8 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 7.75 | 257.89 | -22.03 | 77.33 | 0.3826 | 725.0 | 536.1 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 7.69 | 251.07 | -28.85 | 79.88 | 0.4877 | 712.0 | 607.8 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 6.87 | 250.07 | -29.85 | 81.77 | 0.5013 | 713.0 | 580.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |